Table 1: Photometric properties of the lens galaxy.
Band Effective radius $R_{\rm e}$ $\langle\mu\rangle^1$ $m_{{\rm tot}}$

[ $^{\prime\prime}$ ] [ h₇₀^-1 kpc] [mag arcsec^-2] [mag]

$R_{\rm c}$ 0.36 $\pm$ 0.05 2.9 $\pm$ 0.4 22.20 $\pm$ 0.10 22.42

i 0.36 2.9 20.70 $\pm$ 0.20 20.92

J 0.41 $\pm$ 0.01 3.3 $\pm$ 0.1 18.64 $\pm$ 0.03 18.58

H 0.43 $\pm$ 0.01 3.4 $\pm$ 0.1 17.70 $\pm$ 0.03 17.54

$K_{\rm s}$ 0.50 $\pm$ 0.01 4.0 $\pm$ 0.1 17.13 $\pm$ 0.03 16.63

¹ $\langle\mu\rangle$ is the average surface brightness, not to be confused with the surface
brightness at the effective radius $\mu(R_{\rm e})=\mu_{{\rm e}}$ .

**Table 1:** Photometric properties of the lens galaxy.
Band	Effective radius $R_{\rm e}$	$\langle\mu\rangle^1$	$m_{{\rm tot}}$
	[ $^{\prime\prime}$ ]	[ h₇₀^-1 kpc]	[mag arcsec^-2]	[mag]
$R_{\rm c}$	0.36 $\pm$ 0.05	2.9 $\pm$ 0.4	22.20 $\pm$ 0.10	22.42
i	0.36	2.9	20.70 $\pm$ 0.20	20.92
J	0.41 $\pm$ 0.01	3.3 $\pm$ 0.1	18.64 $\pm$ 0.03	18.58
H	0.43 $\pm$ 0.01	3.4 $\pm$ 0.1	17.70 $\pm$ 0.03	17.54
$K_{\rm s}$	0.50 $\pm$ 0.01	4.0 $\pm$ 0.1	17.13 $\pm$ 0.03	16.63

Source LaTeX | All tables | In the text

	1 Introduction
	2 Modeling the gravitational lensing system
	3 The lens galaxy
	4 The source galaxy
	References